Auriga : The Charioteer

24
Auriga: The Charioteer

description

Auriga : The Charioteer. In Case You’ve Never Seen It Before. An Old Constellation. Gigir “The Chariot” - the name given it in ancient Sumeria between 3500 & 2500BC. Heniochos “The Charioteer” -its classic Greek name. Auriga “The Charioteer” -its latin name from the Romans . - PowerPoint PPT Presentation

Transcript of Auriga : The Charioteer

Page 1: Auriga : The Charioteer

Auriga: The Charioteer

Page 2: Auriga : The Charioteer

In Case You’ve Never Seen It Before..

Page 3: Auriga : The Charioteer

An Old Constellation

•Gigir “The Chariot” - the name given it in ancient Sumeria between 3500 & 2500BC.•Heniochos “The Charioteer” -its classic Greek name. •Auriga “The Charioteer” -its latin name from the Romans.

Page 4: Auriga : The Charioteer

Who’s the Charioteer? Take your pick!

Hephaetus Myrtilus

PoseidonErichthonius

Page 5: Auriga : The Charioteer

…And What’s Up with the Goat?

•Capella, the brightest star, is old Roman for “The She-Goat.”•The Romans recognized Epsilon, Zeta & Eta Aur as “The Kids”•The Greeks only saw two Kids, Zeta & Eta•No mythological basis. Perhaps Mom & the kids are best treated as own asterism.

Page 6: Auriga : The Charioteer

Constellation Facts• Abbreviation: Aur• Coords: RA 6 h Decl: +40° • Area: 657 sq. deg. (21st/88) • Brightest star: Capella (α

Aur) (0.8mag ) • Nearest star: QY Aur (20.0 ly)

Messier objects: 3• Meteor showers: Alpha Aurigids (Aug 25th- Sep 6th))Delta Aurigids (Sept-22 to Oct 23)• Bordered by

CamelopardalisPerseusTaurusGeminiLynx

Page 7: Auriga : The Charioteer

Where’s it at?

Page 8: Auriga : The Charioteer

Finding It: Winter Hexagon

From Cheryl Haimann’sBackyard Astronomywww.pikerpress.com(Used with permission)

Page 9: Auriga : The Charioteer

Finding It From Orion

From Cheryl Haimann’sBackyard Astronomywww.pikerpress.com(Used with permission)

Page 10: Auriga : The Charioteer

Finding it (cont’d)

Use top 2 stars in Big Dipper’s bowl and head west 70 degrees. You’ll run into Capella

Page 11: Auriga : The Charioteer

The Pentagon, or “Five Chariots”

•Capella (mag 0.8) “She-Goat”, 6th brightest star in the sky•Mankalinan (mag 1.9) “Shoulder of the Reinholder”•Bogardus (2.62)•AlKab( Hassaleh)(2.69)•ElNath (1.6) “Butting One”, technically Beta Tauri

Page 12: Auriga : The Charioteer

Capella- The “She-Goat” is Twins

•Capella a & b are both G-class giants, of around 3 solar masses each. They probably started life on the main sequence as A-class dwarfs, but are early into their red giant phase.•The two suns circle each other at a distance closer than our earth-sun distance (0.73 AU). Their combined luminosity is 150 times our sun.•Capella is circumpolar at our latitude.

Page 13: Auriga : The Charioteer
Page 14: Auriga : The Charioteer

The AntiCenter of our Galaxy is in Auriga

Page 15: Auriga : The Charioteer

Those Wonderful Open ClustersM36,M37,M38

M38

M37

M36

Page 16: Auriga : The Charioteer

AE Aurigae & the Flaming Star Nebula

AE Aur is a “runaway” star ejected from the star-forming region in Orion some 2.7 million years ago. It’s big, young, and bright, and illuminates its current area of space, producing the Flaming Star Nebula (IC 405).

Page 17: Auriga : The Charioteer

Variables in Auriga•Zeta Aurigae is an eclipsing binary. Every 2.6 years, it dims ½ magnitude for 40 days.

•Beta Aurigae (Menkalinan) is an EB too, dimming 0.1 magnitude for 10 hours every 4 days.

•AE Auriga (remember the flame star?) varies between mag 5.8 & 6.1 , being young & wild (INA).

Page 18: Auriga : The Charioteer

Epsilon Aurigae:“This Strange Star”• A Class F Supergiant• First noted to vary in brightness in 1821.• Observations in 1847-48, 1874-75,1901-2

showed it dimming for periods of 2 years! • Hans Ludendorff proposed in 1904 that

Epsilon Aurigae is an Eclipsing Binary with a period of 27.1 years.

• Last eclipse was 1982-84. Next predicted eclipse is 2009-11.

• How can an eclipse take two years?

Page 19: Auriga : The Charioteer

How Eclipsing Binaries Work

• One companion star gets in our line of sight of the other, blocking some part the light we see.

• For this to work for Epsilon Auriga, the occluding star would have to be HUGE- 3000 AU!

• If it’s not a star, how about a disk of matter?

Page 20: Auriga : The Charioteer

The Eclipsing Disk Model

• A disk of matter around the star that’s not in our line of site all of the time, but periodically gets in the way and dims the light we receive.

• There’s still a problem with this model if we look at the light curves from past eclipses…

Page 21: Auriga : The Charioteer

It gets brighter in the middle of the eclipse. We need a hole- a donut?

Page 22: Auriga : The Charioteer

The Current “Orbiting Donut” Model

•Two B- class stars orbit each other, and are surrounded by a big circum-stellar disk. •This young, messy system in turn shares an orbit with our F0 suoergiant primary.•In our line of sight, light can pass through the “transparent” B stars in the middle of the eclipse.

Page 23: Auriga : The Charioteer

Watch for it !•First Contact August 6 2009 (est)•Midoint Aug 10 2010 (est)•Done May 15 2011 (647 Days total)

0.1

3.2 3.8

2.7

2.8-?

Page 24: Auriga : The Charioteer

Resources

• American Association of Variable Star Observers: http://www.aavso.org

• Epsilon Aurigae Campaign Page: http://www.hposoft.com/Astro/PEP/EpsilonAurigae.html

• IYA 2009 Epsilon Aurigae Project: http://astronomy2009.us/citizen_science/epsilon-aurigae/

• Feb 2009 Sky & Telescope Celestial Calendar Column

That’s It!!!